Pith. sign in

Paper Citation Record · LEDGER

Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1410.7398.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1410.7398 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:22:54.496123Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-06-29T02:13:00.453011Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 22753bfe-aa79-429d-b555-b5f30df52daa · inbound

CSST Preparations: Galaxy Completeness and S\'ersic Profile Fitting across the Wide, Deep, and Extreme Fields cites this paper.

CSST Preparations: Galaxy Completeness and S\'ersic Profile Fitting across the Wide, Deep, and Extreme Fields Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-11T22:26:14.132877Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-05-08T02:46:19.282636Z digest=sha256:a475b1d36328612a21fd04b92ac57de8639f6114ed2150c5654de9671d9fdaa7

Observation c7b3c702-d662-484e-a399-8c61c3d49e13 · inbound

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations cites this paper.

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Reference 123

Resolution
verified exact
local_arxiv, observed 2026-06-25T23:48:43.294710Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6a18152fb658541202ffc03c595dfbd26f2380e39aa801e1f521c98b1446c313

Observation 908584e8-ef0f-4d42-b247-e87c8a7a4bde · inbound

Quantifying the inside-out formation of disk galaxies at $1.5 \le z \le 3.0$ cites this paper.

Quantifying the inside-out formation of disk galaxies at $1.5 \le z \le 3.0$ Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-06-26T01:38:51.019220Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ccad95e791453ced7e1bcafcc2bc7bc8cdf48aca791e0929dd171efda2c3d427

Observation bf0f82c6-2584-4eae-bfbd-6bc2ed61474a · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-06-29T02:13:00.454339Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d56393a03ade45a8683c018d18536e4662ce521f40ca85cf8b7b9cf00883ea31

Observation bf567528-4f18-4e36-aab6-620f846934f9 · inbound

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium cites this paper.

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Reference 153

Resolution
unresolved
no resolver link, observed 2026-08-02T02:22:54.496123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:22:54.496123Z digest=sha256:3d784c8fb6a6619397737ff12f77e75ffb8cb040a9da816a19fb20b8c9a92e87